arXiv Analytics

Sign in

arXiv:2012.10669 [astro-ph.HE]AbstractReferencesReviewsResources

Testing General Relativity with NuSTAR data of Galactic Black Holes

Ashutosh Tripathi, Yuexin Zhang, Askar B. Abdikamalov, Dimitry Ayzenberg, Cosimo Bambi, Jiachen Jiang, Honghui Liu, Menglei Zhou

Published 2020-12-19Version 1

Einstein's theory of General Relativity predicts that the spacetime metric around astrophysical black holes is described by the Kerr solution. In this work, we employ state-of-the-art in relativistic reflection modeling to analyze a selected set of NuSTAR spectra of Galactic black holes to obtain the most robust and precise constraints on the Kerr black hole hypothesis possible today. Our constraints are much more stringent than those from other electromagnetic techniques, and with some sources we get stronger constraints than those currently available from gravitational waves.

Related articles: Most relevant | Search more
arXiv:2010.13474 [astro-ph.HE] (Published 2020-10-26)
Testing the Kerr Black Hole Hypothesis with GX 339-4 by a combined analysis of its thermal spectrum and reflection features
arXiv:2111.00719 [astro-ph.HE] (Published 2021-11-01)
The spins of Galactic black holes from Insight-HXMT
arXiv:2003.09663 [astro-ph.HE] (Published 2020-03-21)
Testing the Kerr black hole hypothesis using X-ray reflection spectroscopy and a thin disk model with finite thickness